Image('../Plots/akari_conf_title.png')
hp.mollview(lfi30ghz,
title = 'Planck Low Frequency Instrument: 30 GHz All-sky map',
norm = 'hist',
cmap = 'rainbow',
unit = '$K_{CMB}$')

https://arxiv.org/abs/1502.01588
Image('../Plots/akari_conf_intro_spinning_dust.png')
Image('../Plots/akari_conf_intro_hensley.png')
Image('../Plots/akari_conf_intro_irc9.png')
Image(filename = PATH + "/png/band-ratio-G100.png")
Image('../Plots/png/AMEvsDust_allsky_allbands__mpsub_kde.png')
Image('../Plots/png/AMEvsDust_allsky_allbands__mpsub__UNorm_kde.png')
IR Bands' Intensity and AME
Image('../Plots/png/all_bands_corr_matrix_wAME_spearmanintensity.png')
Image('../Plots/png/all_bands_corr_matrix_wAME_spearmanU_norm.png')
Image('../Plots/Allsky_Corr/Spearman_Map_nside8_A9toAME.png')
Image('../Plots/Allsky_Corr/Spearman_Map_nside8_A140toAME.png')
Image('../Plots/Allsky_Corr/RadNorm/Spearman_Map_nside8_A9toAME.png')
Image('../Plots/png/LOri_akari9_AMEcont_1dres.png')
Image('../Plots/lOrionis_grid_img.png')
Spearman Correlation Matrix
Image('../Plots/png/Allsky_corr_Lori.png')
18 micron to 65 micron bands correlate the worst? AME apparently weaker at higher $T_{dust}$ pixels Destruction of PAHs in the center? Something else? ..stay tuned for dust SED modeling (with help from F. Galliano)
Image('../Plots/png/Lori_A9I12.png')